Jökull

Ataaseq assigiiaat ilaat

Jökull - 01.12.1984, Qupperneq 55

Jökull - 01.12.1984, Qupperneq 55
1971), and they are evidently due to Antarctic volcanoes (Kyle and Jezek 1978). Why is this so and why are such tephra layers not present in Greenland ice cores? — There seem to be only two logical explanations of this fact: 1) The many volcanic eruptions during the Holocene did not produce sufficiently large amounts of fine tephra to add significantly to the Greenland dust concentrations. 2) Greenland is too far “down-wind” from “close” eruption sites as compared to Antarc- tica. The geographical position of Antarctica at higher latitudes than the southern polar frontal system and a rather circumpolar movement of the debris laden airmasses secures a much higher chance for fine tephra of “local” origin to remain in the dry Antarctic air. With respect to fine tephra from distant erup- tions the only major difference between Green- land and Antarctica, (to judge from fission-pro- duced radioactive material from the nuclear bomb tests during the years 1953-1965, especially Sr90), is a 2-3 times higher concentration in East Antarctica due to the low level of the yearly precipitation, (H.B. Clausen personal com- munication, 1983). The absence of visible ash layers in the Greenland Ice Sheet must therefore be due to both point 1 and 2. If tephra is taken as a general term for fine volcanic debris, it would include the acid volcanic gases; in fact I can quote Sigurður Thorarinsson (1981, p. 133) “Tephrochronological connections have through the work on Greenland ice cores, become global. . .” Using the word tephra in this sense, acid tephra layers can be detected in the ice sheets. Before discussing the acid volcanic layers in the Greenland Ice Sheet a few remarks on the only visible dust layer of atmospheric “origin”, observed in Greenland ice cores would be in place. A VISIBLE DUST LAYER IN THE DYE 3 CORE A visible yellow to brown banded layering, a few cm thick was observed in the Dye 3 deep core. It was preceded (in time) by a 30 cm annual ice layer (from summer to summer) of more than 50 times the average Holocene dust concentra- tion. Other visible layers exist in the core, but they are near to the bedrock and consist of bot- tom derived material. The layer was encountered at 751,51 meters depth and is a statistical anomaly, when com- pared to Holocene dust concentrations in Green- land ice cores. The layer is indicated in Fig. 1 (left side). The seasonal ð(lsO) variation over the year of high dust deposition showed no unusual varia- tion, which suggests, that no unusual meteorological pattern, at least in the Greenland region, was the cause of the high dust concentra- tion. The electrical conductivity was below nor- mal and pH measurements proved the layer to be neutral or even slightly alkaline: The latter being unique for Holocene ice, at least over an entire annual ice layer. An inspection of the dust by SEM, TEM and microprobe techniques revealed layered as well as unlayered microcrystalline material of high Si content. Uncalibrated microprobe data give the following area percentage of the Ka spectrum, accelerator voltage 21—26 kV: Si:69.3 Al:1.9 K:5.8 Fe:19.2 Ca:0.6 If the layer is a tephra layer it deserves some attention, because it is dated to 174—175 A.D., which is not too far from the 14C date 130 A.D. for the New Zealand Taupo eruption which has been suggested as the cause of unusual atmos- pheric optical phenomena during the reign of the Chinese emperor Ling Ti — A.D. 168—189 (Wil- son et al. 1980). Wilson et al. quote the Chinese annals: “During the reign of Ling Ti several times the Sun rose in the east red as blood and lacking light, only when it had risen to an elevation of more than two zhang was there any brightness. When it set in the west, at two zhang above the horizon it was similarly red. — Also during this period, several times when the Moon rose and set and was two to three zhang above the horizon, all was red as blood”. (A zhang is approximately equal to 12°) The low conductivity of the debris layer could be due to the special eruptive type of Taupo, but there are complications in interpreting the layer as volcanic! — Why is there no similar visible layer in the Antarctic Byrd core; after all the JÖKULL 34. ÁR 53
Qupperneq 1
Qupperneq 2
Qupperneq 3
Qupperneq 4
Qupperneq 5
Qupperneq 6
Qupperneq 7
Qupperneq 8
Qupperneq 9
Qupperneq 10
Qupperneq 11
Qupperneq 12
Qupperneq 13
Qupperneq 14
Qupperneq 15
Qupperneq 16
Qupperneq 17
Qupperneq 18
Qupperneq 19
Qupperneq 20
Qupperneq 21
Qupperneq 22
Qupperneq 23
Qupperneq 24
Qupperneq 25
Qupperneq 26
Qupperneq 27
Qupperneq 28
Qupperneq 29
Qupperneq 30
Qupperneq 31
Qupperneq 32
Qupperneq 33
Qupperneq 34
Qupperneq 35
Qupperneq 36
Qupperneq 37
Qupperneq 38
Qupperneq 39
Qupperneq 40
Qupperneq 41
Qupperneq 42
Qupperneq 43
Qupperneq 44
Qupperneq 45
Qupperneq 46
Qupperneq 47
Qupperneq 48
Qupperneq 49
Qupperneq 50
Qupperneq 51
Qupperneq 52
Qupperneq 53
Qupperneq 54
Qupperneq 55
Qupperneq 56
Qupperneq 57
Qupperneq 58
Qupperneq 59
Qupperneq 60
Qupperneq 61
Qupperneq 62
Qupperneq 63
Qupperneq 64
Qupperneq 65
Qupperneq 66
Qupperneq 67
Qupperneq 68
Qupperneq 69
Qupperneq 70
Qupperneq 71
Qupperneq 72
Qupperneq 73
Qupperneq 74
Qupperneq 75
Qupperneq 76
Qupperneq 77
Qupperneq 78
Qupperneq 79
Qupperneq 80
Qupperneq 81
Qupperneq 82
Qupperneq 83
Qupperneq 84
Qupperneq 85
Qupperneq 86
Qupperneq 87
Qupperneq 88
Qupperneq 89
Qupperneq 90
Qupperneq 91
Qupperneq 92
Qupperneq 93
Qupperneq 94
Qupperneq 95
Qupperneq 96
Qupperneq 97
Qupperneq 98
Qupperneq 99
Qupperneq 100
Qupperneq 101
Qupperneq 102
Qupperneq 103
Qupperneq 104
Qupperneq 105
Qupperneq 106
Qupperneq 107
Qupperneq 108
Qupperneq 109
Qupperneq 110
Qupperneq 111
Qupperneq 112
Qupperneq 113
Qupperneq 114
Qupperneq 115
Qupperneq 116
Qupperneq 117
Qupperneq 118
Qupperneq 119
Qupperneq 120
Qupperneq 121
Qupperneq 122
Qupperneq 123
Qupperneq 124
Qupperneq 125
Qupperneq 126
Qupperneq 127
Qupperneq 128
Qupperneq 129
Qupperneq 130
Qupperneq 131
Qupperneq 132
Qupperneq 133
Qupperneq 134
Qupperneq 135
Qupperneq 136
Qupperneq 137
Qupperneq 138
Qupperneq 139
Qupperneq 140
Qupperneq 141
Qupperneq 142
Qupperneq 143
Qupperneq 144
Qupperneq 145
Qupperneq 146
Qupperneq 147
Qupperneq 148
Qupperneq 149
Qupperneq 150
Qupperneq 151
Qupperneq 152
Qupperneq 153
Qupperneq 154
Qupperneq 155
Qupperneq 156
Qupperneq 157
Qupperneq 158
Qupperneq 159
Qupperneq 160
Qupperneq 161
Qupperneq 162
Qupperneq 163
Qupperneq 164
Qupperneq 165
Qupperneq 166
Qupperneq 167
Qupperneq 168
Qupperneq 169
Qupperneq 170
Qupperneq 171
Qupperneq 172
Qupperneq 173
Qupperneq 174
Qupperneq 175
Qupperneq 176
Qupperneq 177
Qupperneq 178
Qupperneq 179
Qupperneq 180
Qupperneq 181
Qupperneq 182
Qupperneq 183
Qupperneq 184
Qupperneq 185
Qupperneq 186
Qupperneq 187
Qupperneq 188
Qupperneq 189
Qupperneq 190
Qupperneq 191
Qupperneq 192
Qupperneq 193
Qupperneq 194
Qupperneq 195
Qupperneq 196

x

Jökull

Direct Links

Hvis du vil linke til denne avis/magasin, skal du bruge disse links:

Link til denne avis/magasin: Jökull
https://timarit.is/publication/1155

Link til dette eksemplar:

Link til denne side:

Link til denne artikel:

Venligst ikke link direkte til billeder eller PDfs på Timarit.is, da sådanne webadresser kan ændres uden advarsel. Brug venligst de angivne webadresser for at linke til sitet.